
Dominik Schleicher
Computational Astrophysics Group
Contact: dschleicher (at) astro-udec.cl
Research interests
Formation of supermassive black holes via direct collapse
We explore the formation of supermassive black holes via the direct collapse scenario, which assumes that a large fraction of a massive gas cloud collapses into one single object. Our goal is to quantify the conditions when this is feasible, considering the possibility of fragmentation and subsequent mergers.
Formation of supermassive black holes via collisions
We explore the formation of supermassive black holes via collisions in dense metal-poor stars clusters and nuclear star clusters, including the effects of mass loss due to winds or during collisions. This includes formation mechanisms via black hole clusters embedded in external potentials.
Formation of supermassive black holes in new hybrid scenarios
Our group has developed new hybrid scenarios for the origin of supermassive black holes, considering the interaction of collisions and accretion. We have shown that the number of collisions is enhanced in the presence of gas accretion, potentially leading to the formation of very massive objects.
Accretion and growth of supermassive black holes
Our group explores the accretion and growth of supermassive black holes, both in a cosmological context, but also for nearby low-luminosity AGN to study their potential appearance with the Event Horizon Telescope.
Stellar magnetism
We study the origin of stellar magnetism, including dynamo mechanisms in solar mass stars, M-dwarfs and A-type stars using 3D magneto-hydrodynamical simulations. We are also involved in the analysis of TESS data to derive rotation periods.
Magnetism in stellar binaries
We explore the origin of magnetism and long cycles in Double Periodic Variables (DPVs) and Post-Common-Envelope Binaries. Our group has pursued the first numerical simulations that quantify the changes of the stellar structure and resulting eclipsing time variations due to magnetism.
Group Members

Prof. Dr. Dominik Schleicher
Group Leader
Dr. B. Bandyopadhyay
Postdoc
Dr. R. Riaz
Postdoc
Dr. G.-Y. Zhang
Postdoc
F. Agurto
Master Student
M. Cortez
Master Student
B. Gaete
Master Student
J. Lagunas
Master Student
C. Ortiz
Master Student
J. Pedreros
Master Student
K. Sehlke
Master Student
J. Soto
Master Student
P. Solar
Master Student
C. Villegas
Undergraduate StudentFormer group members
- Patricio Alister, now PhD student at the University of Heidelberg
- Dr. Tjarda Boekholt, now postdoc at the University of Oxford
- Claudio Bravo, now in private sector
- Prof. Dr. Stefano Bovino, now associate professor at the University of Concepcion
- Dr. Pedro Capelo, now postdoc at the University of Zurich
- Vanesa Diaz, now PhD student at the University of Hamburg
- Patricio Fibla, now in private sector
- Dr. Philipp Grete, now Marie-Curie fellow at Hamburg Observatory
- Prof. Dr. Muhammad Latif, now professor at UAE University
- Felipe Navarrete, now PhD student at Hamburg Observatory
- Dr. Tim Lichtenberg, now postdoc at the University of Oxford
- Prof. Dr. Remudin Mekuria, now assistant professor at Addis Ababa University
- Camila Olave, now in private sector
- Dr. Kai Rodenbeck, now postdoc at the Max Planck Institute for Solar System Science
- Ruben San Martin, now in private sector
- Joaquin Zamponi, now PhD student at MPE Garching
Third-party funding
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Millennium Nucleus for Transversal Research and Technology to explore Supermassive Black Holes
This project concerns the investigation of the formation, accretion processes and growth of supermassives black holes, as well as site testing and instrumentation efforts for the Event Horizon Telescope. The emphasys of my work concerns black hole formation in different scenarios, as well as the derivation of predictions for the appearance of nearby low-luminosity AGN for the Event Horizon Telescope.
Role: Alternate Director
Project Number: NCN19 508
Website -
Fondecyt regular "Eclipsing time variations in post-common-envelope binaries: planetary hypothesis vs magnetic activity"
This project concerns the investigation of the origin of eclipsing time variations in post-common-envelope binaries, considering magnetic activity as well as planetary companions. We specifically perform 3D magneto-hydrodynamical simulations that quantify how much the stellar structure and as a result the binary orbit can be affected by the dynamo.
Role: Principal Investigator
Project Number: 1201280
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Host Professor Fondecyt postdoctorado
Projects led by Bidisha Bandyopadhyay and Rafeel Riaz
Organization of conferences and schools
- KROME Computational Schools, last version online, 22.02.-05.03.2021
- Supermassive Black Holes Conference, online, December 7-11 2020
- First Stars VI conference, Concepción, March 2-6 2020
- XIV Annual Meeting 2017 of the Chilean Astronomical Society (SOCHIAS), Marbella Resort, January 23-26 2017
- The low-metallicity ISM: Chemistry, Turbulence and Magnetici Fields, Goettingen, October 8-12 2012